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Magnetic fields inferred by Solar Orbiter: A comparison between SO/PHI-HRT and SDO/HMI

Authors :
Sinjan, Jonas
Calchetti, Daniele
Hirzberger, Johann
Kahil, Fátima
Valori, Gherardo
Solanki, Sami K.
Albert, Kinga
Albelo Jorge, Nestor
Álvarez Herrero, Alberto
Appourchaux, Thierry
Bellot Rubio, Luis Ramón
Blanco Rodríguez, Julián
Feller, A.
Gandorfer, Achim
Germerott, Dietmar
Gizón, Laurent
Gómez Cama, José María
Guerrero, Lucas
Gutiérrez Marques, Pablo
Kolleck, Martin
Korpi Lagg, Andreas
Michalik, Harald
Moreno Vacas, Alejandro Miguel
Orozco Suárez, David
Pérez Grande, Isabel
Sanchis Kilders, Esteban
Balaguer Jiménez, María
Schou, Jesper
Schühle, Udo
Staub, Jan
Strecker, Hanna María
Del Toro Iniesta, José Carlos
Volkmer, Reiner
Woch, Joaquim
Sinjan, Jonas
Calchetti, Daniele
Hirzberger, Johann
Kahil, Fátima
Valori, Gherardo
Solanki, Sami K.
Albert, Kinga
Albelo Jorge, Nestor
Álvarez Herrero, Alberto
Appourchaux, Thierry
Bellot Rubio, Luis Ramón
Blanco Rodríguez, Julián
Feller, A.
Gandorfer, Achim
Germerott, Dietmar
Gizón, Laurent
Gómez Cama, José María
Guerrero, Lucas
Gutiérrez Marques, Pablo
Kolleck, Martin
Korpi Lagg, Andreas
Michalik, Harald
Moreno Vacas, Alejandro Miguel
Orozco Suárez, David
Pérez Grande, Isabel
Sanchis Kilders, Esteban
Balaguer Jiménez, María
Schou, Jesper
Schühle, Udo
Staub, Jan
Strecker, Hanna María
Del Toro Iniesta, José Carlos
Volkmer, Reiner
Woch, Joaquim
Publication Year :
2023

Abstract

Context. The High Resolution Telescope (HRT) of the Polarimetric and Helioseismic Imager on board the Solar Orbiter spacecraft (SO/PHI) and the Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO) both infer the photospheric magnetic field from polarised light images. SO/PHI is the first magnetograph to move out of the Sun–Earth line and will provide unprecedented access to the Sun’s poles. This provides excellent opportunities for new research wherein the magnetic field maps from both instruments are used simultaneously. Aims. We aim to compare the magnetic field maps from these two instruments and discuss any possible differences between them. Methods. We used data from both instruments obtained during Solar Orbiter’s inferior conjunction on 7 March 2022. The HRT data were additionally treated for geometric distortion and degraded to the same resolution as HMI. The HMI data were re-projected to correct for the 3° separation between the two observatories. Results. SO/PHI-HRT and HMI produce remarkably similar line-of-sight magnetograms, with a slope coefficient of 0.97, an offset below 1 G, and a Pearson correlation coefficient of 0.97. However, SO/PHI-HRT infers weaker line-of-sight fields for the strongest fields. As for the vector magnetic field, SO/PHI-HRT was compared to both the 720-second and 90-second HMI vector magnetic field: SO/PHI-HRT has a closer alignment with the 90-second HMI vector. In the weak signal regime (< 600 G), SO/PHI-HRT measures stronger and more horizontal fields than HMI, very likely due to the greater noise in the SO/PHI-HRT data. In the strong field regime (≳600 G), HRT infers lower field strengths but with similar inclinations (a slope of 0.92) and azimuths (a slope of 1.02). The slope values are from the comparison with the HMI 90-second vector. Possible reasons for the differences found between SO/PHI-HRT and HMI magnetic field parameters are discussed.<br />BMWi - Bundesministerium für Wirtschaft und Energie (Alemania)<br />AEI/MCIN/10.13039/501100011033<br />Ministerio de ciencia e innovación de España<br />Instituto Astrofísico de Andalucía (España)<br />Agencia Estatal de Investigación (España)<br />Fondo Europeo de Desarrollo Regional (Fondos FEDER)<br />Centre national d'études spatiales (CNES) (Francia)<br />CSIC (Centro Superior de Investigaciones Científicas) (España)<br />Sección Deptal. de Óptica (Óptica)<br />Fac. de Óptica y Optometría<br />TRUE<br />pub

Details

Database :
OAIster
Notes :
application/pdf, 0004-6361, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1450537328
Document Type :
Electronic Resource